In this section, we extend the magnetized Reissner-Nordstrom /CFT correspondence reported in [1]} to the case with the presence of NUT parameter. The first step is to obtain the near horizon geometry for a MRNTN black hole, which can be achieved by performing the transformation
\(t \rightarrow \frac{{r_0 t}}{\lambda }~~,~~r \rightarrow r_e + \lambda r_0 r~~,~~\phi \rightarrow \phi + \Omega _J^{ext} \frac{{r_0 }}{\lambda }t\,.\) 
